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Rejuvenated Accretors Have Less Bound Envelopes: Impact of Roche Lobe Overflow on Subsequent Common Envelope Events

  • Authors: M. Renzo, E. Zapartas, S. Justham, K. Breivik, M. Lau, R. Farmer, M. Cantiello, B. D. Metzger

M. Renzo et al 2023 The Astrophysical Journal Letters 942 .

  • Provider: AAS Journals

Caption: Figure 8.

Ratio of binding energy of a nonrotating 18 M model (left) or of our 15 → 18 M accretor (right) divided by the binding energy of the rotating models of Figure 7. The binding energy includes the internal energy (α th = 1); the gray bands highlight the CEB region of the models in the numerator. Lighter colors indicate ratios to an initially faster-rotating single star; see also legend in Figure 7.

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